Transparency

Economic information: Grants

Awarded

To see the Grants awarded by the IAC (Access the National Subsidy Advertising System) select "Convocatorias", Admon. del Estado: select:  Ministerio de Ciencia, Innovación e Universidades;  Organo: select: Instituto de Astrofísica de Canarias

Received

  • comPact Objects Kinematics, stEllar populations and their Black hOLes in a multiWaveLength approach
    Early Type Galaxies (ETGs) are a key component of the Universe, as they contain most of its stellar mass. They are known to follow many scaling relations, mostly driven by the massive end. The ETGs can be split into two distinctive realms: the already well-known, well-studied extended realm (formed by large ETGs and dwarf galaxies) and a relatively
    Anna
    Ferré Mateu
    In force date
    Not in force
  • Science and technology for the Ariel mission: IAC contribution
    The Atmospheric Remote-sensing Infrared Exoplanet Large-survey (Ariel) mission will address the fundamental questions on what exoplanets are made of and how planetary systems form and evolve by investigating the atmospheres of many hundreds of diverse planets orbiting different types of stars. This large and unbiased survey will contribute to
    Enric
    Pallé Bago
    In force date
    Not in force
  • Nominative grant for the excecution of the Cosmolab 2024 project
    CosmoLAB is a project of the Institute of Astrophysics of the Canary Islands in collaboration with the Cabildo of Tenerife, whose objective is to encourage the educational community of the island to identify the scientific culture, the sky of the Canary Islands and its observatories as part of its own natural heritage and cultural. Within the
    Verónica María
    Martín Jiménez
    In force date
    Not in force
  • Temporal Evolution of the Milky-way Properties from an Observational and theoretical Sinergy (GA 101066193)


    Understanding how galaxies form and evolve in the Universe is a key, long-term goal of Astrophysics. In this regard, our Galaxy provides unique insights because, due to its proximity, detailed galactic properties can be resolved that can unravel its formation history. For this reason, the international community and in particular European countries
    María Alejandra
    Martín Gálvez
    In force date
    Not in force
  • The Multiple Early Channels of EvolutioN of mAssive Stars
    Massive stars are those with more than ~8 solar masses, the limit above which stars may undergo a core collapse supernova (SN) explosion at the end of its life. They have played a critical role in how the Universe has evolved and to understand this role we need to know the physics ruling them and the evolutionary paths they follow. In the last
    Artemio
    Herrero Davo
    In force date
    Not in force
  • Numerical invetigation of the environment and evolution of galaxies
    Cosmological simulations of galaxy formation have increasingly become instrumental tools in advancing our understanding of structure formation in the Universe. Such simulations follow the nonlinear evolution of galaxies by modelling the essential physical processes involved in galaxy formation over a huge range of temporal and spatial scales
    Christopher
    Brook
    In force date
    Not in force